Anomalous dimensions and non-gaussianity

被引:0
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作者
Daniel Green
Matthew Lewandowski
Leonardo Senatore
Eva Silverstein
Matias Zaldarriaga
机构
[1] Stanford University,Stanford Institute for Theoretical Physics
[2] SLAC National Accelerator Laboratory,School of Natural Sciences
[3] Kavli Institute for Particle Astrophysics and Cosmology,undefined
[4] CERN,undefined
[5] Theory Division,undefined
[6] Institute for Advanced Study,undefined
关键词
Cosmology of Theories beyond the SM; Conformal and W Symmetry;
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摘要
We analyze the signatures of inflationary models that are coupled to interacting field theories, a basic class of multifield models also motivated by their role in providing dynamically small scales. Near the squeezed limit of the bispectrum, we find a simple scaling behavior determined by operator dimensions, which are constrained by the appropriate unitarity bounds. Specifically, we analyze two simple and calculable classes of examples: conformal field theories (CFTs), and large-N CFTs deformed by relevant time-dependent double-trace operators. Together these two classes of examples exhibit a wide range of scalings and shapes of the bispectrum, including nearly equilateral, orthogonal and local non-Gaussianity in different regimes. Along the way, we compare and contrast the shape and amplitude with previous results on weakly coupled fields coupled to inflation. This signature provides a precision test for strongly coupled sectors coupled to inflation via irrelevant operators suppressed by a high mass scale up to ~ 103 times the inflationary Hubble scale.
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